Paper
29 June 2000 Probing black hole x-ray binaries with the Keck telescopes
Emilios T. Harlaftis, Alex V. Filippenko
Author Affiliations +
Abstract
The advent of the large effective apertures of the Keck telescopes has resulted in the determination with unprecedented accuracy of the mass functions and mass ratios of faint x-ray transients as well as constraining the main- sequence companion star parameters and producing images of the accretion disks around the black holes.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Emilios T. Harlaftis and Alex V. Filippenko "Probing black hole x-ray binaries with the Keck telescopes", Proc. SPIE 4005, Discoveries and Research Prospects from 8- to 10-Meter-Class Telescopes, (29 June 2000); https://doi.org/10.1117/12.390146
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Cited by 1 scholarly publication.
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KEYWORDS
Stars

X-rays

X-ray telescopes

Doppler effect

Absorption

Telescopes

X-ray astronomy

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